The environmental effect on galaxy evolution: Cl J1449 + 0856 at z = 1.99
2020 ◽
Vol 15
(S359)
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pp. 170-172
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AbstractThis work focuses on understanding the formation of the first massive, passive galaxies in clusters, as a first step to the development of environmental trends seen at low redshift. Cl J1449 + 0856 is an excellent case to study this - a galaxy cluster at redshift z = 1.99 that already shows evidence of a virialised atmosphere. Here we highlight two recent results: the discovery of merger-driven star formation and highly-excited molecular gas in galaxies at the core of Cl J1449, along with the lowest-mass Sunyaev-Zel’dovich detection to date.
2012 ◽
Vol 8
(S292)
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pp. 199-208
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2019 ◽
Vol 485
(3)
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pp. 3409-3429
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2020 ◽
Vol 498
(2)
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pp. 1560-1575
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2019 ◽
Vol 15
(S352)
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pp. 350-352
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2015 ◽
Vol 11
(S315)
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pp. 199-206
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2019 ◽
Vol 15
(S352)
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pp. 281-281
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2008 ◽
Vol 4
(S256)
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pp. 215-226
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